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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-05-12T03:48Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-05-12T03:48:00-CME-001 (version 1)
Note Keyword:
3P: 3-part structure CME
Source Signature Keyword:
OFL: Moving/Opening field lines
Morphology Keyword:
F: Flux Rope
Note: This wide flux rope CME is seen to the SW in all three coronagraphs. The source is field line movement and ejecta from well beyond the SW limb: field line movement visible starting around 2024-05-12T02:49Z in SDO AIA 193; some ejecta seen from beyond the SW limb in SDO AIA 304 starting around 02:20Z; ejecta, filamentary material, and moving field lines visible at 03:33Z in SDO AIA 171.

Submitted on 2024-05-12T13:09Z by Hannah Hermann

A Notification with ID 20240512-AL-001 was sent on 2024-05-12T13:30Z

The List of CME Analysis already entered:
Event Type Catalog
Measurement TypeCME measurement type: Leading Edge (LE), Shock Front (SH), Right Hand Boundary (RHB), Left Hand Boundary (LHB), Black/White Boundary (BW), Prominence Core (COR), Disconnection Front (DIS), Trailing Edge (TE).
Prime?"primary flag" which is either True or False. If there are multiple CME analysis entries for a single CME, this flag would indicate which analysis is considered most accurate per measurement type. This is a helpful flag if you would like to download only one most accurate CME analysis per CME per Measurement Type
 Technique Long Lat Speed Type Half Width Time 21.5 Note WSA-ENLIL+Cone Result(s) Submitted By
CME Analysis M2M_CATALOG LE true SWPC_CAT 137.0 -39.0 602.0 C 47.0 2024-05-12T10:09Z Measurement using farsided source parameters based on source signatures in UV imagery, as well as best 3D fit between coronagraphs. 1: Result 1 (2.0 AU)
Mars = 2024-05-15T22:00Z
OSIRIS-APEX = 2024-05-14T20:00Z
Parker Solar Probe = 2024-05-14T06:00Z
Solar Orbiter = 2024-05-14T14:00Z
Hannah Hermann on 2024-05-12T13:11Z



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